Measurements of the Reaction Rate Coefficients of Atomic Hydrogen with Astrochemical Anions: CN− and C3N−

Christine Lochmann, Sruthi Purushu Melath, Robert Wild, Ersin Yurtsever, Alberto Martín Santa Daría, Lola González-Sánchez, Francesco A. Gianturco and Roland Wester
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Abstract

We present the temperature-dependent reaction rate coefficients of CN− and C3N− with atomic hydrogen in the temperature range from 7 to 290 K, measured in a 16-pole radio-frequency ion trap. The rate of C3N− with H steadily increases toward lower temperatures, while the rate coefficients for the CN− + H system show a sudden change around 160 K. Fits to the data were performed to determine temperature-dependent reaction rate coefficients. The fits reveal a rate coefficient of cm3 s−1 for C3N− + H. For CN−, we determined a rate coefficient for the temperature regime below 160 K of cm3 s−1. Given our present results, higher rate coefficients than previously reported must be assumed for the modeling of cold interstellar environments involving these H atom reactions.
原子氢与天体化学阴离子反应速率系数的测量:CN- 和 C3N-
我们展示了在 16 极射频离子阱中测量到的 CN- 和 C3N- 与原子氢在 7 至 290 K 温度范围内随温度变化的反应速率系数。C3N- 与氢的反应速率随着温度的降低而稳步上升,而 CN- + H 系统的速率系数则在 160 K 附近出现了突变。拟合结果表明,C3N- + H 的速率系数为 cm3 s-1。对于 CN-,我们确定了 160 K 以下温度下的速率系数为 cm3 s-1。鉴于我们目前的结果,在对涉及这些 H 原子反应的寒冷星际环境建模时,必须假设比以前报告的更高的速率系数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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